International Centre for Radio Astronomy Research

The International Centre for Radio Astronomy Research (or ICRAR) is an international centre of excellence in astronomical science and technology, launched in 2009 as a joint venture between Curtin University and the University of Western Australia.[1][2][3] ICRAR attracts some of the world's leading researchers in radio astronomy, contributing to Australian and international scientific and technical programs for the international Square Kilometre Array (SKA) project, the world's biggest ground-based telescope array which is in its design phase and the two Australian SKA precursors, the Australian Square Kilometre Array Pathfinder (ASKAP) and the Murchison Widefield Array (MWA), both located at Murchison, Western Australia. The headquarters of ICRAR are located in Crawley, Western Australia.

Aims

ICRAR was created to deliver world-class outcomes for science, engineering and high performance computing and to play a key role in the SKA. It seeks to:

Participants

ICRAR is an equal joint venture between Curtin University and The University of Western Australia, with funding support from the State Government of Western Australia. The Centre’s headquarters are located at UWA, with research nodes at both UWA and the Curtin Institute for Radio Astronomy (CIRA).

Research

(information to be provided)

Management

ICRAR is governed by a board, chaired by Dr. Bernard Bowen, (appointed in February 2009).[4] The Executive Director is Professor Peter Quinn.[5]

Pawsey Centre

In 2013, ICRAR became the first user of the Pawsey Super-Computing centre, based in Kensington, Western Australia.[6]

theSkyNet

As part of its programme, ICRAR utilises distributed computing to support its own resources. TheSkyNet POGS[7] is a public research project that employs Internet-connected computers to do research in astronomy using BOINC technology. It is currently combining the spectral coverage of GALEX, Pan-STARRS1, and WISE to generate a multi-wavelength (ultra-violet - optical - near infra-red) galaxy atlas for the nearby Universe. It calculates physical parameters such as: star formation rate, stellar mass of the galaxy, dust attenuation, and total dust mass of a galaxy; on a pixel-by-pixel basis using spectral energy distribution fitting techniques. In September 2014 theSkyNet had 13573 users with credit and 5198 users with recent credit[8]

References

External links

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